Metallicity of the star HD80290(F3V)

  • Z. A. Samedov
  • G. M. Hajiyeva
  • Z. F. Aliyeva
  • N.H. Samedova


The atmospheres of the HD80290(F3V) star of the F spectral class were studied using the model and parallax methods. The effective temperatures Teff and surface of gravity g of stars were determined based on a comparison of the observed and theoretically calculated values of the photometric quantity [c1] and the equivalent widths of the spectral lines of the hydrogen Balmer series and the use of parallax. Based on the FeII lines, the microturbulence

How to Cite
SAMEDOV, Z. A. et al. Metallicity of the star HD80290(F3V). Astronomy & Astrophysics (CAUCASUS), [S.l.], v. 5, p. 65-70, sep. 2022. ISSN 2449-2914. Available at: <>. Date accessed: 06 oct. 2022.